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Stellar HostProfile

TOI-7510

G3 • 249.0 pc

Records

6

literature rows

Planets

3

system count

References

5

distinct source labels

TIC: TIC 118798035

Approximate color

from effective temperature

Canonical Summary

Adopted host values from one source row

Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.

Stellar source: Almenara et al. 2025 • System source: TICv8

Temperature

5720 K

5586 to 5820

6 values • 3 distinct

Mass

1.06 Msun

0.99 to 1.06

3 values • 3 distinct

Radius

1.03 Rsun

1.02 to 1.08

6 values • 3 distinct

Luminosity

0.01 log(Lsun)

-0.01 to 0.01

3 values • 3 distinct

Distance

249.0 pc

single adopted value

6 values • 1 distinct

Spectral Type

G3

Consistent across records

G3 (1)

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 1.03 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-7510

1.03 R☉

System Layout

Known planets

3 planets linked to this host

TOI-7510 b

Transit

◌

Discovery

2025

Period

11.53 days

Radius

7.31 R⊕

Mass

18.10 M⊕

Eq. Temp

878 K

TOI-7510 c

Transit

◌

Discovery

2025

Period

22.57 days

Radius

10.81 R⊕

Mass

131 M⊕

Eq. Temp

702 K

TOI-7510 d

Transit

◌

Discovery

2025

Period

48.86 days

Radius

10.52 R⊕

Mass

190 M⊕

Eq. Temp

542.4 K

TOI-7510: A Sun-Like Star With Three Jupiter-Like Worlds

TOI-7510 is a G3 star located 812 light-years away. Its mass is 1.06 solar masses, its radius is 1.03 solar radii, and its temperature is 5720 K. The star's reported radius estimate is larger than the Sun's, but its reported temperature is cooler than the Sun's. Three planets orbit this host.

All three planets are Jupiter-like, a size class that exceeds 4 times Earth's radius. Each was discovered by transit, the method that detects a planet passing in front of its star and causing a small dip in observed brightness.

TOI-7510 b has a mass of 18.1 Earth masses, a radius of 7.31 Earth radii, and an orbital period of 11.5 days. Among the listed planets, it has the shortest year, the smallest radius, and the smallest reported mass. Its mean density is 0.255 g/cm³, 0.0463 times Earth's.

TOI-7510 c has a mass of 131 Earth masses, a radius of 10.8 Earth radii, and an orbital period of 22.6 days. Among the listed planets, it has the second-shortest year, the largest radius, and the second-smallest reported mass. Its mean density is 0.571 g/cm³, 0.104 times Earth's.

TOI-7510 d has a mass of 190 Earth masses, a radius of 10.5 Earth radii, and an orbital period of 48.9 days. Among the listed planets, it has the longest year, the second-smallest radius, and the largest reported mass. Its mean density is 0.899 g/cm³, 0.163 times Earth's.

Each planet's reported radius and mass estimates are larger than Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

6

Stellar refs

4

System refs

1

Distancestable

6 values • 1 distinct

Parallaxstable

6 values • 1 distinct

Temperaturedisputed

6 values • 3 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

6 values • 3 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

6 values • 3 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5586—1.08———249.0ExoFOPTICv8
55860.991.08—9.14e-3—249.0TICv8TICv8
5586—1.08———249.0ExoFOPTICv8
5586—1.08———249.0ExoFOPTICv8
58201.021.024.40-0.01—249.0Brahm et al. 2025TICv8
57201.061.03—0.01G3249.0Almenara et al. 2025TICv8